Corner plots of the central stellar velocity dispersion, σ₀, and truncation radius, r_t, for two cluster members (38 729 on the left and 34 423 on the right) in A2744, obtained from the inference procedure. The posterior probability distributions of σ₀ and r_t and their correlations are shown. The median values and percentiles are highlighted as in Fig. 4. The r_t posterior probability distributions for these galaxies are classified as flat and tailed, respectively. The σ₀ posterior distribution is close to a Gaussian distribution for both galaxies.